Non-Singular Solution of General Relativity Theory Equations

The centric and symmetric solution of equations of Einstein field with potential g₄₄ = -exр(-2r₀r^-1) is examined. Non-singular but quite realistic metric with non-standard signature is obtained where there is no place for "black holes". The space suffers compression in angular co-ordinates and extension in r. However the extension is directed not outwards but inwards, towards the source of field-mass, and so the system is stable.